The SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback
APPROVED PROPOSALS
SINFONI Survey for Unveiling the Physics and the Effect of Radiative feedback (SUPER), PI V. Mainieri, SINFONI/VLT Large Programme, 196.A-0377, 280 hours
SUPER-ALMA: gas fractions and depletion timescales in AGN hosts at z~2, PI V. Mainieri, ALMA Cycle-4, Band-3, 2016.1.00798.S, 13 hours
SUPER-ALMA v2: gas fractions and depletion timescales in AGN hosts at z~2, PI V. Mainieri, ALMA Cycle-5, Band-3, 2017.1.00893.S, 20 hours
SUPER-APEX: Molecular gas properties in X-ray selected AGN at z~2, PI C. Cicone, SHFI/APEX, 098.A-0774, 20 hours
Detecting the molecular CGM around an AGN at z=2, PI V. Mainieri, ALMA/ACA Cycle-7, 2019.2.00118.S, 15 hours
Verifying molecular gas depletion in AGN hosts at z~2, PI C. Circosta, JVLA C-Configuration, VLA/21A-253, 46 hours
Relation between radio properties and ionized gas outflows in high redshift AGN, PI D. Kakkad, JVLA C-Configuration, VLA/21A-256, 36 hours
A missing piece of the puzzle: the warm molecular phase of AGN-driven outflows at Cosmic Noon, PI V. Mainieri, JWST Cycle-1 GO-2177, MIRI/MRS, 13 hours
JWST/MIRI unravels the impact of AGN feedback on star-formation at cosmic noon, PI V. Mainieri, JWST Cycle-2 GP-3158, MIRI/MRS, 19 hours
A systemic search for warm molecular gas in AGN and star forming galaxies at z=2 with MIRI, PI D. Kakkad, JWST Cycle-2 GO-3257, MIRI/MRS, 26 hours